Open Access

Table B.1.

Model atoms used in the CMFGEN calculations.

Ion NSL Nfull Last level Nlines
He I 40 51 n = 11 716
He II 13 30 n = 30 813
C I 14 26 2s 2p33Po 229
C II 14 26 2s2 4d 2D 181
C III 62 112 2s 8f1Fo 1 788
N I 44 104 2s2 2p2(3P)5f 2Fo 1 678
N II 23 41 2s2 2p 3d 1Po 276
N III 25 53 2s 2p(3Po)3d 4Do 523
O I 21 51 2s2 2p3(4So)4f 3F 439
O II 54 123 2s2 2p2(3P)4f 2Fo 2 677
O III 44 86 2s 2p2(4P)3p 3Po 1 017
Ne I 78 155 2s2 2p5(2P3/2)6f 2[7/2] 3 581
Ne II 22 91 2s2 2p4(3P)4d 2P 2 143
Ne III 32 80 2s2 2p3(4So)4f 3F 860
Na I 22 71 30w2W 3 128
Mg II 31 80 30w 2W 3 863
Mg III 31 99 2p5 7s 1Po 1 526
Al II 26 44 3s 5d1D 333
Al III 27 60 10z 2Z 1 191
Si II 31 59 3s2 7h 2Ho 1 059
Si III 33 61 3s 5g3G 615
Si IV 37 48 10f 2Fo 816
S II 56 324 3s 3p3(5So)4p 6P 16 965
S III 48 98 3s 3p2(2D)3d 3P 1 714
S IV 27 67 3s 3p(3Po)4p 2D 1 091
Ar I 56 110 3s2 3p5(2P3/2)7p 2[3/2] 3 030
Ar II 134 415 3s2 3p4(3P1)7i 2[6] 40 224
Ar III 32 346 3s2 3p3(2Do)8s 1Do 13 681
Ca II 21 77 3p6 30w 2W 3 365
Ca III 16 40 3s2 3p5 5s 1Po 210
Ca IV 18 69 3s 3p5(3Po)3d 4Do 647
Sc II 38 85 3p6 3d 4f 1Po 1 905
Sc III 25 45 7h 2Ho 454
Ti II 37 152 3d2(3F)5p 4Do 13 413
Ti III 33 206 3d 6f 3Ho 9 485
Cr II 28 196 3d4(3G)4p x4Go 8 249
Cr III 30 145 3d3(2D2)4p 3Do 4 996
Cr IV 29 234 3d2(3P)5p 4Po 12 569
Mn II 25 97 3d4(5D)4s2 c5D 464
Mn III 30 175 3d4(3G)4p y4Ho 6 292
Fe I 44 136 3d6(5D)4s 4p x5Fo 3 934
Fe II 228 2 698 3d5(4F)4s 4p b4Go 1 062 164
Fe III 96 1 001 3d5(6S)6f 7Fo 138 327
Fe IV 100 1 000 3d4(3G)4f 4Po 144 005
Fe V 139 1 000 3d2(3P)4s 4p 3So 144 265
Co I 52 327 3d7 4s(5F)4d f4H 23 067
Co II 112 1 005 3d7(4P)4f b5Go 205 747
Co III 88 1 075 3d6(3H)4f 4Go 154 662
Co IV 56 1 000 3d5(2D)5s 1D 139 240
Ni I 56 301 3d9(2D5/2)7d 2[7/2] 22 065
Ni II 59 1 000 3d8(3F)7f 4Io 103 224
Ni III 47 1 000 3d7(2D)4d 3S 132 677
Ni IV 54 1 000 3d6(5D)6p 6Fo 145 745
Ni V 54 1 000 3d4(1I)4s21I 151 806
Total 2 613 17 996 2 739 134

Notes: Due to a gf cut (level dependent, gf > 5 × 10−4) only 672 614 lines were included in the non-LTE calculations of the level populations. 1 373 191 lines were included when computing the observed spectrum.

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